Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minute to calcaulte
Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
6.4071 -44.2362 0.0046 30.3592 -164.5732 3.4011525 42.035 TRIG_01418729
Foreground time interval of the image:
-15.136 14.565 (delta_t = 29.701 [sec])
Background time interval of the image:
-239.136 -15.136 (delta_t = 224.000 [sec])
Lightcurves
Notes:
- 1) The mask-weighted light curves are using the flight position.
- 2) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
- 3) For all the mask-weighted lightcurves, the y-axis units are counts/sec/det where a det is 0.4 x 0.4 = 0.16 sq cm.
- 4) The verticle lines correspond to following: green dotted lines are T50 interval, black dotted lines are T90 interval, blue solid line(s) is a spacecraft slew start time, and orange solid line(s) is a spacecraft slew end time.
- 5) Time of each bin is in the middle of the bin.
1 s binning
From T0-310 s to T0+310 s
From T100_start - 20 s to T100_end + 30 s
Full time interval
64 ms binning
Full time interval
From T100_start to T100_end
From T0-5 sec to T0+5 sec
16 ms binning
From T100_start-5 s to T100_start+5 s
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
8 ms binning
From T100_start-3 s to T100_start+3 s
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
2 ms binning
From T100_start-1 s to T100_start+1 s
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
SN=5 or 10 sec. binning (whichever binning is satisfied first)
SN=5 or 10 sec. binning (T < 200 sec)
Quad-rate summed light curves (from T0-300s to T0+1000s)
Spectral Evolution
Spectra
Notes:
- 1) The fitting includes the systematic errors.
- 2) When the burst includes telescope slew time periods, the fitting uses an average response file made from multiple 5-s response files through out the slew time plus single time preiod for the non-slew times, and weighted by the total counts in the corresponding time period using addrmf. An average response file is needed becuase a spectral fit using the pre-slew DRM will introduce some errors in both a spectral shape and a normalization if the PHA file contains a lot of the slew/post-slew time interval.
- 3) For fits to more complicated models (e.g. a power-law over a cutoff power-law), the BAT team has decided to require a chi-square improvement of more than 6 for each extra dof.
Time averaged spectrum fit using the average DRM
Power-law model
Time interval is from -15.136 sec. to 288.864 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.56085 ( -0.0844344 0.0846945 )
Norm@50keV : 1.51141E-03 ( -7.00912e-05 6.99074e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.22 using 59 bins.
Reduced chi-squared = 1.03895
# Null hypothesis probability of 3.95e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 304 sec: 0.191947 ( -0.00928 0.009311 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.31951e-06 ( -2.14407e-07 2.15142e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -15.136 sec. to 288.864 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.48168 ( -0.329681 0.155406 )
Epeak [keV] : 338.281 ( -338.313 -338.313 )
Norm@50keV : 1.65258E-03 ( -0.000204571 0.000719416 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.03 using 59 bins.
Reduced chi-squared = 1.05411
# Null hypothesis probability of 3.65e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 304 sec: 0.191044 ( -0.009913 0.009479 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.29403e-06 ( -2.36857e-07 2.2696e-07 ) ergs/cm2
Band function
Time interval is from -15.136 sec. to 288.864 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 15.2586 ( )
R^2/D10^2 : 1.95953E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 178.85 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.68e-14 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.895e-07 2.874e-08
25- 50 1.168e-06 7.509e-08
50-150 1.865e-06 1.628e-07
15-150 3.323e-06 1.870e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-37.7528 -200)
Norm : 0.776413 (-0.0353983 0.0353983)
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.49 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.51e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.885e-07 2.918e-08
25- 50 1.132e-06 5.913e-08
50-150 2.483e-06 1.257e-07
15-150 4.203e-06 2.295e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.87946 (-1.16097 1.27704)
R1^2/D10^2 : 0.217659 (-0.0946681 0.207709)
kT2 [keV] : 26.8370 (-4.01722 6.35178)
R2^2/D10^2 : 2.16993E-03 (-0.00113687 0.00177995)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.67 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.75e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.733e-07 9.819e-08
25- 50 1.120e-06 1.389e-07
50-150 2.559e-06 4.580e-07
15-150 4.252e-06 5.670e-07
Peak spectrum fit
Power-law model
Time interval is from 8.364 sec. to 9.364 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.29803 ( -0.329198 0.322741 )
Norm@50keV : 7.50870E-03 ( -0.00141287 0.00140906 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.46 using 59 bins.
Reduced chi-squared = 1.11333
# Null hypothesis probability of 2.59e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.895494 ( -0.172711 0.173296 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.42438e-08 ( -1.53065e-08 1.55011e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 8.364 sec. to 9.364 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.891918 ( -1.59667 1.63985 )
Epeak [keV] : 142.702 ( -142.699 -142.699 )
Norm@50keV : 1.18616E-02 ( -0.00563996 0.0566429 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.14 using 59 bins.
Reduced chi-squared = 1.1275
# Null hypothesis probability of 2.39e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.881191 ( -0.179223 0.178439 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.2282e-08 ( -1.68194e-08 1.64152e-08 ) ergs/cm2
Band function
Time interval is from 8.364 sec. to 9.364 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 16.9504 (-3.72558 5.32328)
R^2/D10^2 : 6.97722E-02 (-0.0420764 0.0943083)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.05 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.50e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.086e-09 1.459e-09
25- 50 1.804e-08 5.634e-09
50-150 3.697e-08 1.533e-08
15-150 5.909e-08 2.213e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-78.1552 -200)
Norm : 3.72238 (-0.704258 0.704258)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.89 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.21e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.270e-09 5.430e-09
25- 50 1.783e-08 1.009e-08
50-150 3.911e-08 2.271e-08
15-150 6.621e-08 3.780e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.79145 (-7.4155 -9.79163)
R1^2/D10^2 : 0.297447 (-0.223103 78.7125)
kT2 [keV] : 37.3051 (-34.9315 -37.3061)
R2^2/D10^2 : 3.75511E-03 (-0.00369805 0.0615573)
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.19 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.09e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.473e-09 3.901e-09
25- 50 1.864e-08 1.125e-08
50-150 4.819e-08 2.663e-08
15-150 7.330e-08 3.659e-08
Pre-slew spectrum (Pre-slew PHA with pre-slew DRM)
Power-law model
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.28456 ( -0.0662884 0.0658663 )
Norm@50keV : 7.62959E-03 ( -0.000283125 0.000283065 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.09 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.85e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 29.7 sec: 0.907691 ( -0.0360203 0.0360943 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.24776e-06 ( -8.86714e-08 8.88265e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.978576 ( -0.269463 0.253298 )
Epeak [keV] : 185.302 ( -61.3431 517.052 )
Norm@50keV : 1.05435E-02 ( -0.00241806 0.00334291 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.77 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.08e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 29.7 sec: 0.893083 ( -0.037861 0.03791 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.21095e-06 ( -9.49776e-08 9.45945e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 1.10e-06
S(50-100 keV) = 1.49e-06
T90 vs. Hardness ratio plot
T90 = 160 sec.
Hardness ratio (energy fluence ratio) = 1.35455
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.23643
Count Ratio (50-100 keV) / (15-25 keV) = 0.927213
Mask shadow pattern
IMX = -5.646359361218204E-01, IMY = 1.558106563529533E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
Spacecraft aspect plot
Bright source in the pre-burst/pre-slew/post-slew images
Pre-burst image of 15-350 keV band
Time interval of the image:
-239.136000 -15.136000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
14.5610 8.1057 2.6 29.6 69.7 2.1341 4.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-15.136000 14.564600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
34.9798 -3.2609 2.8 40.1 106.9 1.2350 4.2 ------ UNKNOWN
32.1847 -32.1942 2.3 37.0 154.1 0.6080 5.1 ------ UNKNOWN
6.4071 -44.2362 0.3 30.4 -164.6 3.4009 42.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
81.764600 711.997300
720.864000 782.912500
840.864000 962.925100
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
Plot creation:
Sun Mar 1 23:12:10 EST 2026